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The performance of the present interferometers using resonant cavities is continually improving and prospects for the detection of predicted sources of radiation with interferometers of longer baselines seem most encouraging.
In this paper we discuss the use of laser interferometry with resonant optical cavities to sense very small displacements of suspended test masses in a gravitational radiation detector. In particular we describe and discuss the performance of a prototype interferometer currently under development, which has high finesse cavities, 10-m long, and is illuminated by highly frequency-stabilized light from...
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